Detecting exoplanets with the false inclusion probability - Comparison with other detection criteria in the context of radial velocities

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Table 4

Parameters of the different runs of POLYCHORD on the HD 10180 dataset when using a Gaussian mixture prior on semi-amplitude.

Planets	log(Z)	σ_log(Z)	PNP	Runtime
0	−882.45	0.23	3.82e–108	17 s
1	−839.36	0.19	1.08e–93	1 min 56 s
2	−789.03	0.24	3.72e–76	6 min 57 s
3	−736.95	0.04	1.19e–57	17 min 39 s
4	−677.56	0.15	7.27e–36	38 min 41 s
5	−603.42	0.13	1.12e–07	1 h 33 min 31 s
6	−590.14	0.30	6.60e–02	4 h 46 min 46 s
7	−587.49	0.22	9.34e-01	14 h 59 min 57 s

Notes. For a given number of planets in the model (Col. (1)) we performed three runs. The other columns give the log Bayesian evidence (log(Z), median), the standard deviation of log(Z) amongst runs (σ_log(Z)), the PNP, and the runtime.

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